Observation

Observation Details

EIS: Chromosphere corona connection, line asymmetry due to spicule type

2010-06-10T12:28:14 to 2010-06-10T13:30:10

Science Goal: Fast small raster cotemporal with SOT high cadence H-alpha, Ca II

Program:

Target:

xcen=813 ycen=-294

Instrument: EIS

HOP/JOP: 159

Description: STUD_ACR: VHH_HI_BRT_SCAN
FILENAME: eis_l0_20100610_122814.fits

Annotations:

Chief Observer

See also

Datasets

saaIntervals hiIntervals

wavelength: FeXIII cadence: fov: 5,240 images: null
wavelength: SiX cadence: fov: 5,240 images: null
wavelength: CaXVII cadence: fov: 5,240 images: null
wavelength: SiVII cadence: fov: 5,240 images: null
wavelength: HeII cadence: fov: 5,240 images: null
wavelength: FeXII cadence: fov: 5,240 images: null
wavelength: FeXIV cadence: fov: 5,240 images: null

wavelength: FeXIII cadence: fov: 5,240 images: null

wavelength: SiX cadence: fov: 5,240 images: null

wavelength: CaXVII cadence: fov: 5,240 images: null

wavelength: SiVII cadence: fov: 5,240 images: null

wavelength: HeII cadence: fov: 5,240 images: null

wavelength: FeXII cadence: fov: 5,240 images: null

wavelength: FeXIV cadence: fov: 5,240 images: null